The galaxy presents as a relatively compact, elliptical-like structure with a bright, concentrated core. There appears to be a discernible, though faint, disk-like component surrounding the central bulge. The light distribution is smooth, with no readily apparent spiral arm structures or distinct star-forming regions. The color gradient indicates a population of older stars, particularly within the bulge, characterized by redder hues. The presence of a green-ish glow is an indicator of specific elements such as oxygen being present, a sign of star formation. There are no significant signs of ongoing major mergers or tidal disruptions; however, the slightly irregular shape suggests that minor interactions cannot be ruled out. The overall appearance suggests a transitionary stage, potentially an early-type spiral or a late-stage elliptical galaxy that has largely ceased active star formation.
