The galaxy appears as a well-defined, luminous object with a generally smooth morphology. The overall shape is elliptical, showing a high degree of roundness rather than a highly elongated or cigar-like form. There is no readily apparent central bulge, bar, or spiral arm structure. The light distribution appears fairly uniform across the galaxy's surface, with a slight concentration towards the core, but without distinct knots or clumps that would indicate ongoing star formation regions. There is no obvious visual evidence of tidal tails or other signs of major interactions, such as a recent merger event, although there may be a very minor disturbance present. The galaxy's color seems relatively uniform, presenting a yellowish hue, which would be consistent with a stellar population dominated by older stars.
