The galaxy presents an elliptical morphology, appearing somewhat elongated in shape, though not extremely so. Its light profile suggests a relatively smooth distribution, indicating a lack of prominent spiral arms or distinct features typically associated with disk galaxies. The central bulge appears prominent and is characterized by a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluer light extends from the core and appears more patchy and diffused, particularly at the edges. This could indicate more recent star formation activity in these regions. There is a subtle hint of possible minor disturbance within the galaxy's overall structure, which could be evidence of a past or ongoing minor merger event.
