The galaxy presents as a relatively compact object, exhibiting a predominantly smooth morphology. It appears somewhat elliptical in shape, deviating noticeably from a perfectly circular form. The color profile suggests the presence of an older stellar population, indicated by the slightly redder hue. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy shows a marginal degree of disturbance, and a small portion has a more blue hue, potentially indicating ongoing, but not substantial, star formation activity. There is no definitive evidence of a major merger event or significant tidal interactions, but some asymmetry suggests that a more minor disturbance has occurred. Overall, this galaxy seems to be a relatively quiescent system undergoing only minor gravitational interaction.
