The galaxy exhibits a generally elliptical morphology, appearing elongated rather than perfectly circular. The central region is characterized by a bright, concentrated bulge, indicating a significant stellar population. The galaxy displays a relatively smooth texture, with limited evidence of distinct spiral arms or complex structures. A faint, diffuse disk appears to extend outwards from the central bulge, particularly on one side, showing hints of possible disturbance or interaction. There is evidence of ongoing star formation, based on the color profile, with bluer regions present within the fainter disk, suggestive of the presence of younger, hotter stars. There might be on going merger or recent merger with another galaxy due to the disturbed nature of the disk and the slight irregularities in the galaxy's overall shape.
