The galaxy presents an overall elliptical morphology, appearing elongated in shape. The light distribution is concentrated towards the center, with a smooth, diffuse appearance indicative of an older stellar population. The color profile displays a redder hue at the core, suggesting a higher density of evolved stars and dust obscuration within the central region. Moving outward from the center, there is a subtle shift towards slightly bluer colors, potentially indicating the presence of younger star formation in the outer regions, though these are subtle. There are no clearly discernible spiral arm structures or other distinct features such as prominent dust lanes. The galaxy shows no significant signs of major disturbances or ongoing mergers; any disturbances appear minor. The galaxy is moderately sized and rather luminous.
