The galaxy presents as a relatively compact object with a concentrated central bulge. The overall morphology leans toward a prolate spheroid, appearing elongated rather than perfectly circular. While a distinct disk component isn't readily apparent, there's a suggestion of subtle, less-defined structure extending from the core region. The light distribution appears smooth, with a gradual falloff from the bright center. The colour profile indicates a dominant population of older stars in the central region, contributing to the yellowish hue. Faint hints of bluer emission are observable in the outer regions, possibly indicative of more recent star formation activity, or possibly the scattering of light. There is no obvious visual evidence of major merger events. The galaxy appears to be moderately massive.
