The galaxy exhibits a generally smooth morphology with a noticeable elliptical shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The central region appears yellowish-orange, suggesting a population of older stars and a possible lack of significant ongoing star formation. There is a slight elongation or cigar-shaped appearance to the galaxy, indicating that it is not perfectly circular. No distinct spiral arms or prominent dust lanes are visible in this image. There is no evidence of any major mergers or significant tidal disturbances affecting its structure. The outer regions are faint, gradually fading into the background sky.
