The galaxy presents as a single, centrally concentrated object with an overall smooth appearance, though subtle features are present. The primary body exhibits a roughly elliptical morphology, leaning toward round, with no distinct spiral arm structures visible. The light profile appears relatively even, suggesting a lack of significant ongoing star formation or large-scale dust lanes. The galaxy exhibits an orange-red hue, potentially indicating a population of older stars and a lower rate of current star formation. There is possible minor disturbance in the overall structure, but further investigation is needed to confirm any interactions or merging events. No clear evidence of a central bar or bright nucleus is immediately apparent.
