The galaxy appears as an elliptical or lenticular type. It exhibits a smooth, centralized light distribution, with a pronounced bulge region. The overall shape is somewhat elongated, suggesting a possible classification leaning towards an E4-E6 on the Hubble sequence, possibly even an S0 type.  There is little evidence of spiral arms or distinct star-forming regions. The galaxy's color profile indicates a redder hue, indicative of an older stellar population and relatively low ongoing star formation activity. This suggests a galaxy that has likely consumed a significant portion of its gas reservoir, leading to a decline in star formation rates. There is no apparent major mergers or tidal disturbances present.
