The galaxy presents as a relatively smooth, centralized structure, with a notable lack of distinct spiral arms or features. It exhibits a somewhat elliptical morphology, appearing as a flattened spheroid rather than a perfectly circular disk. The concentration of light is brightest toward the center, decreasing outwards with a gradual falloff in surface brightness, indicating a higher density of stars and interstellar material in the central region. There appears to be a slight asymmetry or minor disturbance in the galaxy's overall shape, potentially indicating an ongoing or recent interaction with another galaxy. The galaxy emits light across the visible spectrum, with a slightly stronger presence in the redder bands compared to the bluer bands. This reddening could be due to a higher fraction of older stellar populations, increased dust obscuration, or a combination of both factors. Despite the general smoothness, there may be faint, unresolved knots or clumps within the galaxy, which could represent star-forming regions. However, these are not prominent.
