The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a slight elongation in its overall shape, but it is generally rounded. Its color profile shows a dominant yellow-orange hue, with a subtle shift towards redder tones towards the galactic center. This suggests a population of older stars dominating the light output. There is no obvious presence of spiral arms or significant dust lanes. The galaxy appears to be relatively isolated, with no signs of ongoing major merging activity, although a slight irregularity in its shape hints at a possible past minor interaction. The overall light distribution is quite diffuse, indicating a lack of prominent, actively star-forming regions.
