The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape, with a high degree of central concentration. The central region exhibits a brighter, more luminous core, suggesting the presence of an older stellar population. Fainter, diffuse light extends outwards from the center, showing a gradual decrease in intensity. Hints of what could be a disk or spiral arms are subtly present; a subtle blue hue distributed somewhat irregularly which may indicate regions of more recent star formation or a more substantial disk component than initially implied. No obvious signs of ongoing major mergers or significant tidal disturbances are apparent, although there are suggestions of minor interactions. Overall, this galaxy seems to be moderately massive, with what may be an intermediate star formation rate.
