The galaxy appears as a relatively smooth, elliptical-shaped object with a concentrated central bulge. The core exhibits a bright, yellowish hue, indicating a population of older stars. Moving outwards from the core, the light gradually fades, suggesting a decreasing stellar density. The outer regions possess a more reddish tinge, potentially due to dust absorption or a higher proportion of older, redder stars in the periphery. There are no distinct spiral arm structures or prominent dust lanes visible. The galaxy seems fairly undisturbed, with no major morphological irregularities indicative of recent mergers or tidal interactions. It's moderately sized, appearing neither exceptionally large nor unusually compact.
