This galaxy appears to be a relatively luminous, early-type galaxy, likely an elliptical or lenticular. It exhibits a smooth, centrally concentrated light distribution, with a notable absence of distinct spiral arms or prominent dust lanes. The galaxy displays a moderate ellipticity, appearing somewhat cigar-shaped. The color profile suggests a dominant population of older stars, with a yellowish-red hue characteristic of evolved stellar populations. There is no obvious sign of any major ongoing merger events, though minor tidal disturbances cannot be ruled out. Overall, the galaxy appears to be a fairly massive and quiescent system, consistent with a low star formation rate.
