The galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology. A smooth and diffuse light profile characterizes the galactic structure, with no readily apparent spiral arms or distinct features. The color gradient suggests a population dominated by older stars, with a subtle shift towards bluer hues in the central regions. The overall impression is that of a relatively quiescent system, with limited evidence of ongoing star formation activity. There are some minor disturbances present, hinting at a possible past or ongoing interaction.
