The galaxy presents as a single, relatively smooth, luminous structure with an overall elliptical morphology. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity outwards from the core. There is little evidence of spiral arms, dust lanes, or other distinct morphological features typically associated with disk galaxies. The galaxy appears slightly elongated, deviating subtly from a perfectly circular shape. The galaxy's color profile appears relatively uniform, with a general tendency towards redder hues, suggestive of an older stellar population and potentially lower ongoing star formation activity. There is no indication of any major merger events or significant tidal disturbances in this particular view.
