The galaxy appears to be a relatively bright, early-type system, likely an elliptical, exhibiting a generally smooth morphology. Its color is predominantly yellow-orange, suggestive of an older stellar population. The galaxy appears quite round, with no obvious major disk-like structure. There may be a minor indication of some interaction, which is supported by the presence of a slight disturbance in its otherwise smooth profile, although this could be related to the image quality. The galaxy's overall luminosity suggests it is a massive system. The low star formation rate would also support the notion of an elliptical galaxy composed of aging stars. There is a potential merger or tidal feature, which could be the result of a previous or ongoing interaction.