The galaxy presents as a reddish, elongated spheroid. It exhibits a relatively smooth, homogenous light distribution with no distinct spiral arms, bar structures, or prominent dust lanes visible. The overall color suggests a population dominated by older stars and relatively low star formation activity. There is a subtle hint of bluer light in some regions, possibly indicating pockets of recent star formation, though these are not prominent. The shape suggests the galaxy is likely an elliptical, possibly of type E5-E7, or potentially a lenticular (S0) galaxy viewed nearly edge-on. There appears to be no evidence of ongoing major mergers or tidal disruptions, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated within its immediate environment.
