The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region exhibits a noticeable concentration of light, appearing yellowish in color, suggestive of an older stellar population. The outer regions of the galaxy display a bluer hue, potentially indicating the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. There is no clear evidence of spiral arms or a well-defined disk. Instead, the galaxy appears relatively smooth, though there might be some minor disturbances or irregularities in its overall form. No clear evidence of an ongoing major merger or significant tidal interactions are visible. The estimated mass of the galaxy is quite high, suggesting a mature galaxy with a sizable population of stars.
