The galaxy presents as a single, largely featureless object. Its morphology is primarily smooth and rounded, with a noticeable concentration of light towards the center, suggesting a bulge. There are no visible spiral arms, bars, or prominent dust lanes. The galaxy exhibits a yellowish-white hue, indicative of an older stellar population. The smooth light profile and lack of defined features suggest an elliptical or lenticular classification. There appears to be minimal evidence of ongoing star formation, as indicated by the absence of blue or ultraviolet light and distinct HII regions. No signs of tidal tails, disrupted structures, or nearby companion galaxies are apparent in the immediate vicinity, suggesting it is not currently undergoing a major merger event.
