The galaxy presents as a relatively smooth, centrally concentrated object. The light profile exhibits a gradual falloff from a bright core, indicating a lack of prominent spiral arms or other distinct features. The overall shape appears roughly elliptical, deviating slightly from a perfectly circular morphology, with an estimated effective radius of approximately 3 kpc. The galaxy displays a color gradient, transitioning from a bluer hue in the central regions to redder tones towards the outskirts, possibly indicating differential stellar populations, the central regions appearing to have a more star forming region. Evidence of disturbances and mergers are minimal, suggesting a system that is relatively settled. The mass of the galaxy is estimated to be between 10^8 and 10^9 solar masses. The rate of star formation within the galaxy ranges, suggesting a possible range of activity in this region.
